Shaping HR8799’s outer dust belt with an unseen planet
Author:
Affiliation:
1. Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
2. Department of Physics, University of Warwick, Gibbet Hill Road, Warwick CV4 7AL, UK
Funder
Science and Technology Facilities Council
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/475/4/4953/24062541/sty141.pdf
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1. The Limiting Effects of Dust in Brown Dwarf Model Atmospheres
2. THE CHARA ARRAY ANGULAR DIAMETER OF HR 8799 FAVORS PLANETARY MASSES FOR ITS IMAGED COMPANIONS
3. Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458
4. Oscillations of relative inclination angles in compact extrasolar planetary systems
5. Imaging Young Giant Planets From Ground and Space
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